High-energy neutrino follow-up search of gravitational wave event GW150914 with ANTARES and IceCube

dc.contributor
Centre Tecnològic de Vilanova i la Geltrú
dc.contributor
Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
dc.contributor.author
Adrian Martinez, Silvia
dc.contributor.author
Albert, A.
dc.contributor.author
André, Michel
dc.contributor.author
Anghinolfi, Marco
dc.contributor.author
Anton, G.
dc.contributor.author
Ardid, M.
dc.contributor.author
Aubert, J.-J.
dc.contributor.author
Avgitas, T.
dc.contributor.author
Baret, B.
dc.contributor.author
Barrios Martí, J.
dc.contributor.author
Basa, S.
dc.contributor.author
Bertin, V.
dc.contributor.author
Biagi, S.
dc.contributor.author
Bormuth, R.
dc.contributor.author
Bouwhuis, M.C.
dc.date.issued
2016-06-23
dc.identifier
Adrian-Martinez, S., Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J., Avgitas, T., Baret, B., Barrios, J., Basa, S., Bertin, V., Biagi, S., Bormuth, R., Bouwhuis, M. High-energy neutrino follow-up search of gravitational wave event GW150914 with ANTARES and IceCube. "Physical Review D", 23 Juny 2016, vol. 93, núm. 12.
dc.identifier
0556-2821
dc.identifier
https://hdl.handle.net/2117/90893
dc.identifier
10.1103/PhysRevD.93.122010
dc.description.abstract
We present the high-energy-neutrino follow-up observations of the first gravitational wave transient GW150914 observed by the Advanced LIGO detectors on September 14, 2015. We search for coincident neutrino candidates within the data recorded by the IceCube and ANTARES neutrino detectors. A possible joint detection could be used in targeted electromagnetic follow-up observations, given the significantly better angular resolution of neutrino events compared to gravitational waves. We find no neutrino candidates in both temporal and spatial coincidence with the gravitational wave event. Within +/- 500 s of the gravitational wave event, the number of neutrino candidates detected by IceCube and ANTARES were three and zero, respectively. This is consistent with the expected atmospheric background, and none of the neutrino candidates were directionally coincident with GW150914. We use this nondetection to constrain neutrino emission from the gravitational-wave event.
dc.description.abstract
Postprint (published version)
dc.format
application/pdf
dc.language
eng
dc.publisher
American Physical Society
dc.relation
http://journals.aps.org/prd/abstract/10.1103/PhysRevD.93.122010
dc.rights
http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.rights
Open Access
dc.subject
Àrees temàtiques de la UPC::Física::Acústica
dc.subject
Neutrinos
dc.subject
Neutrino astrophysics
dc.subject
Gamma ray bursts
dc.subject
GAMMA-RAY BURSTS
dc.subject
DATA-ACQUISITION SYSTEM
dc.subject
POINT-LIKE
dc.subject
TELESCOPE
dc.subject
TRANSIENTS
dc.subject
ASTRONOMY
dc.subject
Raigs gamma
dc.subject
Neutrins
dc.title
High-energy neutrino follow-up search of gravitational wave event GW150914 with ANTARES and IceCube
dc.type
Article


Files in this item

FilesSizeFormatView

There are no files associated with this item.

This item appears in the following Collection(s)

E-prints [72987]